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I ntermediate-mass evolved star winds: an observer’s perspective. Jacco van Loon Keele University. Kalirai et al. (2008). Kalirai et al. (2009). Kalirai et al. (2008). A GB. Javadi et al. (2011) (from Marigo et al. 2008). Super - AGB. RSG. Sloan et al. (2009). Sculptor. - PowerPoint PPT Presentation
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Intermediate-mass evolved star winds: an observer’s perspective
Jacco van LoonKeele University
Kalirai et al. (2008)
Kalirai et al. (2009)
Kalirai et al. (2008)
Javadi et al. (2011)
(from Marigo et al. 2008)
AGB
RSG
Super - AGB
Sloan et al. (2009)
Sculptor
Marigo et al. (2008)
Ferrarotti & Gail (2006)
Ferrarotti & Gail (2006)
Ferrarotti & Gail (2006)
Wood et al. (1992)
mass loss
Nguyen et al. (2007)
Croat et al. (2005)
Vollmer et al. (2009)
200 nm
Fe
van Loon et al. (2008)
van Loon et al. (2005)
dust formation radius
maser
Marshall et al. (2004)
Wood et al. (1992)
Marshall et al. (2004)
Atacama Large (sub)Millimeter Array
Australian SKA Pathfinder
CW Leo = IRC +10 216
Leão et al.
Cat’s Eye Nebula
Mira
ω Centauri
Ercole et al. (2012)
2nd generation
pristine gas
1st generation winds
M 4
Ercole et al. (2012)
2nd generation
pristine gas
1st generation winds
NGC 2808
McDonald & van Loon (2007)
McDonald et al. (2009)
Origlia et al.
Reimers
dust
McDonald et al. (2010, 2011)
iron
Sloan et al. (2010)
LMC
SMC
IRAS
Spitzer
van Loon (2006)
Boyer et al. (2012)
Boyer et al. (2012)
Boyer et al. (2012)
Bonanos et al.
(2010)
M 33
2 micron
Spitzer
Javadi et al. (2011)
Javadi et al. (2011)
(from Marigo et al. 2008)
RSG
super-AGB
AGB
AGB super-AGB / RSGRGB
Javadi et al. (2012)
Action points
• Wind kinematics (stellar parameters)• Dust-to-gas ratios (stellar parameters)• Mass-loss rates from not-very-dusty stars• Detailed case studies confronting models…• …and population studies confronting models• Interaction with the ISM and/or companions• Super-AGB stars
Marshall et al. (2004)
van Loon, Marshall & Zijlstra
(2010)
Bonanos et al.
(2010)